More analysis of solar jets/surges, association with the bright points, with spectroscopic techniques to probe the Dopplershifts, bidirectional outflows, and twisting in solar jets are needed to explain their triggering and driving mechanisms. In future, we plan to include the observations from the newly launched Solar orbiter ([1]}; [2]}) and from Swedish 1 m Solar Telescope [3]} to explore the nature of cool and hot jets and their comparison with MHD flux emergence/cancellation models. Such observations can serve to validate the numerical experiments of the theoretical scientists.
